The fast radio burst population energy distribution

Abstract We examine the energy distribution of the fast radio burst (FRB) population using a well-defined sample of 63 FRBs from the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope, 28 of which are localised to a host galaxy. We apply the luminosity-volume ( $V/V_{\mathrm{max}}$ ) test to examine the distribution of these transient sources, accounting for cosmological and instrumental effects, and determine the energy distribution for the sampled population over the redshift range $0.01 \lesssim z \lesssim 1.02$ . We find the distribution between $10^{23}$ and $10^{26}$ J Hz $^{-1}$ to be consistent with both a pure power-law with differential slope $\gamma=-1.96 \pm 0.15$ , and a Schechter function with $\gamma = -1.82 \pm 0.12$ and downturn energy $E_\mathrm{max} \sim 6.3 \, \times 10^{25}$ J Hz $^{-1}$ . We identify systematic effects which currently limit our ability to probe the luminosity function outside this range and give a prescription for their treatment. Finally, we find that with the current dataset, we are unable to distinguish between the evolutionary and spectral models considered in this work.

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Publication Details

Journal
Publications of the Astronomical Society of Australia
Published
2025-01-01
DOI
https://doi.org/10.1017/pasa.2024.114
Citations
7
Primary Topic
Gamma-ray bursts and supernovae
Type
article
Field-Weighted Citation Impact
8.08

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article

The fast radio burst population energy distribution

Chris Flynn, Clancy W. James, R. M. Shannon, W. Arcus et al.
7 citations
Publications of the Astronomical Society of Australia
Gamma-ray bursts and supernovae
8.08
article

The fast radio burst population energy distribution

Chris Flynn, Clancy W. James, R. M. Shannon, W. Arcus, K. W. Bannister, Marcin Glowacki, R. D. Ekers, R. B. Wayth, Jean‐Pierre Macquart, S. D. Ryder, E. M. Sadler, Alexa C. Gordon, Lachlan James Marnoch, Adam T. Deller
article en
7 citations

Abstract

Abstract We examine the energy distribution of the fast radio burst (FRB) population using a well-defined sample of 63 FRBs from the Australian Square Kilometre Array Pathfinder (ASKAP) radio telescope, 28 of which are localised to a host galaxy. We apply the luminosity-volume ( $V/V_{\mathrm{max}}$ ) test to examine the distribution of these transient sources, accounting for cosmological and instrumental effects, and determine the energy distribution for the sampled population over the redshift range $0.01 \lesssim z \lesssim 1.02$ . We find the distribution between $10^{23}$ and $10^{26}$ J Hz $^{-1}$ to be consistent with both a pure power-law with differential slope $\gamma=-1.96 \pm 0.15$ , and a Schechter function with $\gamma = -1.82 \pm 0.12$ and downturn energy $E_\mathrm{max} \sim 6.3 \, \times 10^{25}$ J Hz $^{-1}$ . We identify systematic effects which currently limit our ability to probe the luminosity function outside this range and give a prescription for their treatment. Finally, we find that with the current dataset, we are unable to distinguish between the evolutionary and spectral models considered in this work.

Publications of the Astronomical Society of AustraliaVol. 42
Northwestern University (US), Commonwealth Scientific and Industrial Research Organisation (AU), The University of Sydney (AU), Australia Telescope National Facility (AU), Curtin University (AU), ASTRO-3D (AU), ARC Centre of Excellence for All-sky Astrophysics (AU), International Centre for Radio Astronomy Research (AU), Swinburne University of Technology (AU), Macquarie University (AU)
National Science Foundation, Northwestern University, Science and Industry Endowment Fund, Australian Government, Commonwealth Scientific and Industrial Research Organisation, Government of Western Australia
Affordable and clean energy
Openalex Percentile: Top 3%
Gamma-ray bursts and supernovae
8.08
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